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Table 2
Percentage of test particles representing minor bodies that were discarded from the simulations of both belts due to the minor body collisions with the star and four planets, and due to exceeding the maximum distance from the star with respect to the initial number of test particles.
| Simulation time | Belt | Ejection | Collision | ||||
|---|---|---|---|---|---|---|---|
| Star | e | d | c | b | |||
| 0–70 Myr | Inner | 31% (202 958) | 0.14% (928) | 0.25% (1614) | 0.014% (92) | 0.0068% (44) | 0.0015% (10) |
| Outer | 9.5% (137 143) | 0.014% (208) | 0.0037% (54) | 0.0049% (72) | 0.0077% (112) | 0.041% (595) | |
| 1–70 Myr | Inner | 18% (99 202) | 0.1% (545) | 0.091% (494) | 0.0069% (38) | 0.0039% (21) | 0.00092% (5) |
| Outer | 2.6% (35 205) | 0.0013% (17) | 0.00029% (4) | 0.00069% (9) | 0.00045% (6) | 0.0013% (18) | |
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